Investigation of adsorptive fractionation of humic acid on graphene oxide using fluorescence EEM-PARAFAC

Investigation of adsorptive fractionation of humic acid on graphene oxide using fluorescence EEM-PARAFAC

Accepted Manuscript Investigation of adsorptive fractionation of humic acid on graphene oxide using fluorescence EEM-PARAFAC Bo-Mi Lee, Young-Soo Seo,...

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Accepted Manuscript Investigation of adsorptive fractionation of humic acid on graphene oxide using fluorescence EEM-PARAFAC Bo-Mi Lee, Young-Soo Seo, Jin Hur PII:

S0043-1354(15)00040-8

DOI:

10.1016/j.watres.2015.01.020

Reference:

WR 11112

To appear in:

Water Research

Received Date: 24 September 2014 Revised Date:

9 January 2015

Accepted Date: 10 January 2015

Please cite this article as: Lee, B.-M., Seo, Y.-S., Hur, J., Investigation of adsorptive fractionation of humic acid on graphene oxide using fluorescence EEM-PARAFAC, Water Research (2015), doi: 10.1016/j.watres.2015.01.020. This is a PDF file of an unedited manuscript that has been accepted for publication. As a service to our customers we are providing this early version of the manuscript. The manuscript will undergo copyediting, typesetting, and review of the resulting proof before it is published in its final form. Please note that during the production process errors may be discovered which could affect the content, and all legal disclaimers that apply to the journal pertain.

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Investigation of adsorptive fractionation of humic acid on graphene oxide

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using fluorescence EEM-PARAFAC

Bo-Mi Leea, Young-Soo Seob, and Jin Hura,* a b

Department of Environment and Energy, Sejong University, Seoul, 143-747, South Korea Department of Nano Materials, Sejong University, Seoul, 143-747, South Korea

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Revised and Re-submitted to Water Research, January 2015

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* Corresponding author: Tel. +82-2-3408-3826. E-mail: [email protected]

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Fax +82-2-3408-4320.

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Abstract

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In this study, the adsorptive fractionation of a humic acid (HA, Elliott soil humic acid) on

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graphene oxide (GO) was examined at pH 4 and 6 using absorption spectroscopy and

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fluorescence excitation-emission matrix (EEM)-parallel factor analysis (PARAFAC). The

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extent of the adsorption was greater at pH 4.0 than at pH 6.0. Aromatic molecules within the

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HA were preferentially adsorbed onto the GO surface, and the preferential adsorption was

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more pronounced at pH 6, which is above the zero point of charge of GO. A relative ratio of

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two PARAFAC humic-like components (ex/em maxima at 270/510 nm and at (250, 265)/440

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nm) presented an increasing trend with larger sizes of ultrafiltered humic acid fractions,

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suggesting the potential for using fluorescence EEM-PARAFAC for tracking the changes in

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molecular sizes of aromatic HA molecules. The individual adsorption behaviors of the two

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humic-like components revealed that larger sized aromatic components within HA had a

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higher adsorption affinity and more nonlinear isotherms compared to smaller sized fractions.

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Our results demonstrated that adsorptive fractionation of HA occurred on the GO surface

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with respect to their aromaticity and the sizes, but the degree was highly dependent on

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solution pH as well as the amount of adsorbed HS (or available surface sites). The observed

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adsorption behaviors were reasonably explained by a combination of different mechanisms

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previously suggested.

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Keywords: EEM-PARAFAC; humic substances (HS); graphene oxide (GO); adsorption; size

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fractionation

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1. Introduction Graphene oxide (GO) is a representative form of graphene material that can be easily and cost-effectively obtained in substantial amounts through Hummer’s method (Kowalczuk et al.,

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2010; Yang et al., 2013). GO is a mono-layered material consisting of partially defected

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honeycomb structures containing a portion of various functional groups (e.g., hydroxyl,

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epoxy, carbonyl, and carboxyl groups) (Singh et al., 2011). Owing to its unique structure, GO

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has been used as a precursor material for a number of applications including adsorbents,

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weak cation exchange resin, electrochemical sensors, biosensors, and hydrogen storage

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(Ramesha et al., 2011; Singh et al., 2011; Wang et al., 2009). In the water treatment field,

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much research has been done to utilize GO as an adsorbent for the removal of toxic

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compounds from polluted water (Chowdhury and Balasubramanian, 2014). In addition, GO

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can be easily modified for specific purposes either by transformation of functional groups or

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by composition with nano-particles, or by both (Singh et al., 2011). All of these advantages

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pose GO as one of the most attractive materials for recent environmental applications.

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Although the recent growth of GO usage heightens the probability of exposure to aquatic environments, little attention has been paid to possible environmental significance. For

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example, GO may alter the original water quality by adsorbing certain natural or synthetic

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organic molecules through its large surface (Wang et al., 2014a). The associated adsorption

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mechanisms documented to date are π- π interaction, hydrophobic interaction, and

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electrostatic attraction/repulsion (Apul et al., 2013; Sitko et al., 2013; Zhang et al., 2013;

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Zhao et al., 2012). The sp2 structure, or honeycomb structure, of GO provides a good

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environment for aromatic organics to adsorb through π- π interaction, while the acidic

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functional groups on GO can be responsible for the charge-related adsorption mechanism

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(Wang et al., 2014b). Compared with other carbon nano-materials including reduced GO and

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carbon nanotubes (CNTs), GO can be regarded as a priority material to be examined with

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respect to the environmental significance because it tends to be more dispersed and relatively

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stable in the aqueous phase (Ren et al., 2014; Wang et al., 2014a).

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Humic substance (HS) is a major constituent of naturally occurring organic materials, which are ubiquitously present in aquatic environments. HS is composed of a number of

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aromatic and aliphatic structures of different molecular sizes and functional groups (Bell et

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al., 2014; Hur and Schlautman, 2003). It has been reported that HS structures and their

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composition are closely related to chemical reactivities and the subsequent environmental

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impact (Peña-Méndez, 2005). A well-known functionality of HS is changing the surface

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properties of adsorbents through adsorption (Kungolos et al., 2006; Liang et al., 2007; Weng

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et al., 2006; Yang et al., 2011). The structural heterogeneity of HS can make its adsorption

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behaviors more complicated, possibly leading to preferential adsorption of certain HS

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constituents onto the adsorbent surfaces. There have been previous studies examining HS

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adsorptive fractionation on natural adsorbents (e.g., minerals) and carbonaceous materials

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(e.g., activated carbon) (Alekseeva and Zolotareva, 2013; Hur and Schlautman, 2003; Kang

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and Xing, 2008; Schmit and Wells, 2002). Structural changes of HS upon the adsorption onto

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CNTs were also recently studied by employing various HS characterizing techniques

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including UV absorption spectroscopy and size exclusion chromatography (Wang et al.,

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2011; Yang and Xing, 2009). However, to our best knowledge, there has been no related

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report concerning GO surface, which is unfortunate considering recently growing interest in

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GO and its potentially wide application.

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For the last two decades, the fluorescence excitation-emission matrix (EEM) has been

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established as the most popular tool for tracking the changes in the structures and the

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composition of HS, because of its rapid measurement, non-destructive nature, and high

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sensitivity (Li et al., 2014; Liu et al., 2011; Yamashita, 2008). Combining EEM datasets with

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parallel factor analysis (PARAFAC) has provided even more benefits for tracking the HS 3

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quantitative manner (Cuss and Guéguen, 2012; He et al., 2013; Li et al., 2014; Simon et al.,

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2010; Stedmon and Bro, 2008; Ziegelgruber et al., 2013). Although it looks promising for the

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EEM-PARAFAC to be an excellent technique for exploring the changes of HS upon

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adsorption, there have been only limited studies relying on the EEM-PARAFAC to get insight

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into HS adsorption behaviors. The only precedent was a study of Banaitis et al., (2006), who

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simply compared the relative distributions of four PARAFAC components of soil organic

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matters between before and after adsorption onto minerals.

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This study firstly examined the changes in the characteristics of HS upon the adsorption

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onto GO. The adsorption isotherms and the kinetics were studied at two different pH values

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(4.0 and 6.0) by using absorption spectroscopy and EEM-PARAFAC and focusing on the

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adsorptive fractionation phenomenon. The obtained outcomes can provide a new insight into

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the adsorption behaviors of dissimilar HS components on the GO surface and also into the

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effects of solution pH.

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2. Materials and Methods

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2.1. Preparation of GO

GO was prepared based via a modification of Hummer’s method (Marcano et al., 2010).

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For the preliminary step, 12 g of graphite flakes (Sigma-Aldrich) were oxidized using

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K2SO2 (10 g), P2O5 (10 g) and 50 ml of a concentrated sulfuric acid (95%, Deajung) at 80 oC

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for 5 hours. The pre-oxidized graphite flakes were washed with Milli-Q water and dried in

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ambient conditions. Sodium nitrate (5 g) and dried graphite flakes (10 g) were then mixed in

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a concentrated sulfuric acid (230 ml) at 0 oC. Potassium permanganate (30 g) was added and

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gradually stirred into the mixture, and the solution was kept under 10 oC. The mixture was

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heated to 35 oC and kept for 2 hours before 2 L of Milli-Q water was slowly added and 30% 4

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decanted. The precipitated GO was washed three times with 4 N of HCl to remove

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manganese. The GO solution was then sonicated in the acid condition for 30 minutes in a

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bath sonicator. The GO was finally washed with Milli-Q water to remove acid and the

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possibly remaining impurities that might exist. Single-sheet GO was finally obtained after

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un-exfoliated GO was separated using centrifugation at 5000 rpm for 10 minutes.

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The GO was characterized by scanning electron microscopy (SEM, HITACHI S-4700),

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atomic force microscopy (AFM, Park XE-100), X-ray diffraction (XRD, D/MAX-2500/PC,

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Rigaku), Raman spectroscopy (Renisshaw 633 nm), and Fourier transform infrared

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spectroscopy (FT-IR, Perkin-Elmer spectrum 100). The point of zero charge (pHPZC) of the

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GO was estimated following an acid-base titration method suggested by Li et al. (2012). The

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Brunauer−Emmer−Teller (BET) surface area of the GO is 63.6 m2/g. The GO characteristics

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are described in the support information (Supplementary Information, Table S1; Figs. S1-S6).

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2.2. HS materials

Elliott soil humic acid (ESHA) and Suwannee River fulvic acid (SRFA) were purchased

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from the International Humic Substance Society (IHSS). ESHA was used here as a

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representative humic acid (HA) while SRFA, as a reference material for comparison. The data

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of SRFA are all contained in the Supplementary Information. The aromatic, aliphatic, and

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carboxyl contents are 50%, 16%, and 18%, respectively, for ESHA, and 24%, 33%, and 20%

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for SRFA, respectively, based on 13C-NMR results provided by the IHSS web site

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(www.humicsubstances.org). Using ESHA is beneficial for understanding the complicated

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adsorption behavior of HS in aqueous phase because soil-derived HS has more heterogeneous

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structure than aquatic HS (Hur and Schlautman, 2003).

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2.3. Adsorption kinetics and isotherm experiments Adsorption kinetic experiments were conducted in batch using an initial HS concentration of 15 mgC/L. The solution pH was adjusted to 4.0 and 6.0 by adding 1N NaOH. Different

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amounts of GO were added to the pH-adjusted solutions (300 mg/L and 500 mg/L for pH 4.0

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and 6.0, respectively). The two pH values were selected to investigate the change of

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intermolecular interaction between HS and GO rather than to mimic the natural background

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pH range. It is also noted that the GO concentrations used for this study are much higher than

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the levels that might be encountered in aquatic environments. The mixtures were shaken at a

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room temperature (20±1 oC) on an orbit shaker at 150 rpm for 5 hours in dark.

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Adsorption isotherm experiments were carried out under the same conditions. The added amounts of HS varied from 10 mgC/L to 60 mgC/L in 500 mg/L of the GO suspended

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solution. The equilibrium time was set at 24 hours (Yang et al., 2014a). The variation of the

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pH was minimal during shaking, varying ±0.2 from the original values. Dissolved HS was

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separated from GO-associated fractions using centrifugation at 10,000 rpm, and the

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supernatant was further filtered on a 0.2 µm pre-washed membrane filter (cellulose acetate

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membrane, Advantec). The GO-associated HS or the adsorbed HS fraction was quantified by

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subtracting the concentration of dissolved HS left in the solution from the initial

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concentration.

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Adsorption isotherm parameters were estimated based on two well-known adsorption isotherm models, the Langmuir model (1) and the Freundlich model (2):

Qe =

Qmax kL Ce 1+kL Ce

(1)

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Qe =kF Ce n

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where Qe (mg C/L) and Qmax (mg C/g) are the equilibrium solid-phase concentration and the

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concentration in solution. kL (L/mg C) is the adsorption affinity related to adsorption energy;

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kF and 1/n are the Freundlich model capacity factor and the Freundlich model site

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heterogeneity factor, an indicator of isotherm nonlinearity, respectively.

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The adsorption kinetic parameters were estimated by best fitting the experimental data to a pseudo first order kinetic model (3)

Qt =Qe (1-e-kt t )

(3)

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where Qt and Qe (mg C/g) are the adsorbed amounts of HS after adsorption at the time point t

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and the equilibrium time, respectively. kt (1/h) represents the pseudo first model constant, and

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t is adsorption time (h).

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2.4. Measurements of HS concentrations and the spectroscopic characteristics The initial HS and the residual HS after adsorption were quantified in dissolved organic

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carbon (DOC) concentrations using a TOC analyzer (Shimadzu V-series, TOC-CHP).

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Specific UV absorption (SUVA) values, a rough measure of HS aromaticity, were calculated

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based on DOC concentration-normalized UV absorbance at 254 nm, multiplied by a factor

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of 100. The UV absorbance was obtained using a UV-visible spectrophotometer (HACH,

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DR 5000). Fluorescence EEMs were measured using a luminescence spectrometry (LS-55,

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Perkin-Elmer) by emission scanning between 280 to 550 nm with 0.5 nm increment at the

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excitation wavelengths from 250 to 500 nm at 5 nm-intervals. Excitation and emission slits

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were adjusted at 10 nm, respectively. A 290 nm emission cut-off filter was used to limit

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second-order Raleigh light scattering (Yang et al., 2014b). The scanning speed was set at

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1200 nm/min. Inner-filter correction was made to account for the potential light absorption

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of the HS samples (Gauthier et al., 1986). The obtained fluorescence intensities were

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quinine sulfate dehydrate at an excitation/emission of 350/450 nm. All samples were

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adjusted to the same pH condition (3.0) before the optical measurements, which makes it

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possible to compare the adsorption behaviors at different pH without correcting the potential

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pH-induced changes in HS (Yang and Hur, 2014). The fluorescence response to a blank

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solution (Milli-Q water) was deducted from the measured fluorescence signals of each

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sample.

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2.5. EEM-PARAFAC analysis

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EEM-PARAFAC analysis was conducted using MATLAB 7.1 and the free-download DOMFluor toolbox (www.models.life.ku.dk), following a tutorial of Stedmon and Bro (2003).

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The number of the PARAFAC components was determined by split-half analysis and a core

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consistency test (Supplementary Information, Figs S7 and S8). . The EEM data for the

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PARAFAC modeling were obtained from the HS samples (both ESHA and SRFA) before

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and after adsorption as well as from five ultrafiltered ESHA fractions (the total number = 46).

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2.6. Ultrafiltration of ESHA and the characterization of the HA size fractions In order to obtain the structural and the spectroscopic features of HS changing with the

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sizes, ESHA was separated into five different size fractions using an ultrafiltration process.

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A starting HS solution was prepared by dissolving 220 mg of ESHA in l L of Milli-Q water.

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Ultrafiltration was carried out on an Amicon stirred cell (Amicon 8400) using membranes

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(76 mm, regenerated cellulose, Millipore, Amicon) with different molecular cut-off sizes of

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1, 10, 30, and 100 kDa, which led to five ultrafiltered size fractions of >100 kDa, 30-100

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kDa, 10-30 kDa, 1-10 kDa, and <1 kDa. The different molecular sizes were confirmed by

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employing a size exclusion chromatography system (Waters 1515) equipped with a UV

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was a pH 6.8 phosphate buffer (0.002 M NaH2PO4 and 0.002 M Na2HPO4 in 0.1 M NaCl

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solution) (Hur and Schlautman, 2003). The ESHA fractions were further analyzed by solid

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phase 13C-NMR measurement for the carbon structures (Bruker Avance II). Further details

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of the ultrafiltered size fractions are provided in the supporting information (Supplementary

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Information, Table S2; Figs. S9 and S10).

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3. Results and Discussion

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3.1. Adsorption isotherms of bulk HA on GO surface

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The adsorption isotherms of ESHA are shown in Fig. 1, and the related model parameters are presented in Table 1. The R2 values of the Langmuir and the Freundlich models were all

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high (R2 > 0.86), suggesting that the two isotherm models reasonably explain the adsorption

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behaviors. The Langmuir model parameters theoretically represent the maximum adsorption

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amount (Qmax) and the related adsorption energy or adsorption affinity (kL) under certain

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limited assumptions (i.e., monolayer adsorption, homogeneous surfaces, etc.) (Ren et al.,

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2014), while the Freundlich model is primarily based on an empirical equation to fit the

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adsorption data for heterogeneous surfaces (Allen et al., 2003; Zhang et al., 2013).

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For the bulk HA quantified by DOC measurements, the adsorption affinity (i.e., kL value)

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was higher at pH 4.0 than at pH 6.0 (0.080±0.019 vs. 0.019±0.003 L/mgC). This observation

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may be attributed to the difference in the net surface charge of GO between the pH values.

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Due to the pHPZC of GO (~4.65) (Supplementary Information, Fig. S6), GO is likely to have

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more positively charged (or less negatively charged) surface at pH 4.0 versus 6.0, resulting in

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an elevated contribution of electrostatic attraction to overall adsorption and a lesser extent of

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electrostatic repulsion between the adsorbing HA and GO surface (Moreno-Castilla, 2004).

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Yang et al (2014a) reported a pH-dependent adsorption behavior a peat humic acid on GO,

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Qmax value at a higher pH for this study) (Table 1). A closer examination of the isotherms

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revealed that the adsorbed HA (Qe) at pH 4.0 reached a saturated level at equilibrium HA

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concentrations over 25 mgC/L, ultimately exhibiting more nonlinear adsorption curve

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compared to that at pH 6.0 (0.402±0.064 at pH 4.0 versus 1/n = 0.680±0.031 at pH 6.0; Table

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1, Fig. 1a). The apparent saturation in the adsorption could result from the limitation of the

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GO surface sites available for adsorbing HA. In contrast, relatively more linear sorption

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isotherm at pH 6.0 may be explained by the reduced operation of the site-limiting adsorption

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mechanisms such as electrostatic attraction. Although solution pH also influences the HA

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properties such as the size and the molecular charges, possibly affecting the adsorption

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behaviors, the effects seem to be limited and not strong enough to surpass the pH-induced

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GO changes within the limited pH range of this study. It is because smaller HA size and more

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positive charges on HA at a lower pH would result in a higher Qmax value at pH 4.0 versus 6.0,

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which is the opposite of our results.

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3.2. Adsorption isotherms of HA aromatic molecules on GO surface

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To highlight the adsorption behaviors of aromatic (or UV-absorbing) moieties within HA, the isotherm model parameters were additionally estimated based on UV absorption

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measurements (Table 1; Fig. 1b). High R2 values of the model fit indicate the relevance of the

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isotherm models to describe the data. In this study, a higher R2 value was exhibited for the

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UV-absorbing HS than for the bulk HS (i.e., DOC-based HS) at pH 4.0 but the same R2

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values were found at pH 6.0 (Table 1), supporting that different mechanisms might be

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responsible for the HA adsorption onto GO at the two pH values. Furthermore, a comparison

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of the estimated isotherm parameters between DOC and UV absorption measurements

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showed that the adsorption behaviors of aromatic HA were different from those of the bulk

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ACCEPTED MANUSCRIPT HS. For example, the Qmax value of the UV-absorbing HA was higher and the kL value was

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lower at pH 4.0 than at pH 6.0, while the opposite trend was previously observed for the bulk

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HA (Table 1). In addition, the noticeably limited adsorption sites at a high adsorption amount

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for the bulk HA were not found for this UV-absorbing HA, which exhibited a relatively linear

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isotherm (Table 1, Fig. 1b). These results further imply that the controlling mechanisms for

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the adsorption of aromatic HA molecules may not be the same as those of the bulk HS. The

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adsorption of aromatic HA structures is likely to be much less affected by site-limited

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adsorption mechanisms compared to the bulk HA. This observation appears reasonable

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because π- π interaction, a dominant mechanism, would allow more adsorption sites for

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aromatic HA moieties than for non-aromatic molecules, although further investigation needs

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be warranted for better explanation.

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3.3. Adsorption kinetics of HA onto GO surfaces

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Estimations of adsorption kinetic parameters, based on DOC concentrations, are presented in Table 2. The apparent equilibrium was reached within two hours (Fig. 2), which

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agreed well with a recent report of Yang et al (2014a). The equilibrium concentration (Qe)

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and the adsorption rate (kt) differed at the two pH conditions with the mean values being

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approximately 2.5 and 1.6 times higher at pH 4.0 than at pH 6.0, respectively (Table 2).

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Again, this observation can be explained by the differences in the net surface charges of GO.

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The mean kt values obtained by UV absorption measurements were consistently higher than

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those based on DOC (Table 2), indicating that aromatic HA moieties were adsorbed onto GO

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surface faster than the bulk HA. The relative difference was more pronounced at a higher pH

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(i.e., pH 6.0) where π-π interaction and hydrophobic interaction probably operate to a greater

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extent than electrostatic attraction.

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3.4. Changes in SUVA values upon adsorption The SUVA values of adsorbed ESHA on GO were calculated based on the mass balance between the initial and the residual ESHA after adsorption, and the changes were tracked

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against the adsorption amounts at equilibrium (Fig. 3a) and also with the adsorption time (Fig.

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3b). At the equilibrium condition, the SUVA values of the adsorbed HA were mostly higher

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than the original value, suggesting that aromatic moieties within HA were preferentially

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adsorbed to GO surface. The SUVA values showed an increasing trend with a higher

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adsorption amount at both pH conditions (Fig. 3a). They changed from 8.5 to 10.6 L/mg C-m

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for relatively low adsorption amounts up to ~32 mg C/g at pH 4.0, and from 11.3 to 13.8

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L/mg C-m for all the observed adsorption amounts at pH 6.0. In addition, the differences in

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the SUVA values between the adsorbed and the original HA were consistently larger at pH

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6.0 than at pH 4.0 except for the high adsorption amount above ~32 mg C/g. The relatively

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higher SUVA values indicate that the preferential adsorption of aromatic HA molecules was

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greater at a higher pH where π- π interaction and hydrophobic interaction would be

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predominant. For the range of the adsorbed HS amount above ~32 mg C/g at pH 4.0, the

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SUVA values sharply deviated from a trend with the adsorbed HA amount (Fig. 3a), which

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requires more explanation through further investigations.

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A notable difference was also found for the kinetic changes between the two pH values

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(Fig. 3b). At pH 6.0, the SUVA values of the adsorbed HA were initially much higher than the

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original value and then declined with the adsorption time, varying from 12.0 to 8.7 L/mg C-m.

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Ultimately, the values dropped nearly to the original value. In contrast, no substantial changes

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were observed at pH 4.0 where electrostatic attraction was partially involved. From the

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variation in the kinetics at pH 6.0 and our previous observation of the faster equilibrium for

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the UV-absorbing HA, it can be inferred that the preferential adsorption of HA aromatic

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moieties took place in an early stage of the adsorption, but the adsorbed aromatic molecules

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could be subsequently replaced with non-aromatic structures.

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3.5. PARAFAC components and the relationship with HA molecular size Three different components were successfully decomposed by PARAFAC modeling on

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the EEM data of the samples from the adsorption and the ultrafiltration processes (Fig. 4).

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The core consistency was 96.5% when the three-component model was applied. Several prior

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PARAFAC studies demonstrated that three-PARAFAC component model sufficiently

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described all the fluorescence features of HS (Borisover et al., 2012; Dainard and Guéguen,

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2013; He et al., 2006; Yang and Hur, 2014). The peak of component 1 (C1) was shown at

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relatively longer excitation/emission wavelengths of 270 nm/510 nm, while component 2 (C2)

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had two maxima at shorter wavelengths of 250 nm/440 nm and 265 nm/440 nm. The two

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PARAFAC components can be both assigned to humic-like components. Typically, the

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fluorescence peaks at longer wavelengths (i.e., red-shifting) are associated with structural

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condensation and polymerization of HS (Chen et al., 2003). For instance, Hur and Kim (2009)

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have shown that fluorescence features at longer emission wavelengths were more pronounced

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in the EEMs of larger sized HS fractions. Therefore, the C1 fluorophores probably relate to

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more condensed structures with a larger molecular size than the C2-associated fluorescent

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group. The peaks of component 3 (C3) appeared at <250 nm/365 nm and 290 nm/365 nm,

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which resembled the traditionally-defined aromatic amino acid component (or tryptophan-

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like component). In our study, the majority of fluorescent HS could be described by a

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combination of the two humic-like components, constituting over 80% of the total

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PARAFAC components in the Fmax values (Supplementary Information, Tables S4 and S5).

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ESHA showed a similar relative abundance of C1 and C2 (~48%) in the Fmax values, whereas

353

C2 was more dominant for SRFA with a 70% and 20% relative abundance shown for C2 and

354

C3, respectively (Supplementary Information, Table S4). These results suggest that C2 is

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13

ACCEPTED MANUSCRIPT 355

associated with the presence of fulvic acids, which is known to be less condensed and smaller

356

in size than humic acids (Kang et al., 2002).

357

A plot of the relative ratios of the two humic-like components (i.e., C1/C2) against the weight-average molecular weights (MWw) of the ESHA ultrafiltered size fractions revealed a

359

close association of the ratios with the HA molecular sizes (Fig. 5). The C1/C2 ratios

360

generally increased with the MWw values, indicating that the ratio can be used for tracking

361

the molecular size changes of HA. The relationship was nonlinear (i.e., a concave-down

362

curve), implying that the descriptive capability of the ratio could be limited for relatively

363

large HA molecules (~ >3000 Da).

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364 365 366

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358

3.6. Comparison for the adsorption isotherms between two humic-like components The adsorption isotherms of the two humic-like components (i.e., C1 and C2) were separately examined to explore the individual adsorption behaviors of different components

368

within the bulk HA (Figs. 6a and 6b). Based on the estimated isotherm parameters, the larger

369

sized humic-like component C1 exhibited the lower Qmax and 1/n values, but higher kL and kF

370

values than C2 at both pH conditions (Table 3). Our results indicate that GO has more

371

available sites for C2 than for C1. Considering that the aromatic (or fluorescent) components

372

are mostly attractive to the GO surface through π-π interaction, it is possible to infer that the

373

adsorption of larger sized aromatic molecules might be more limited on the GO surface

374

compared to smaller sized fractions. Furthermore, this tendency was more pronounced at pH

375

4.0, where electrostatic attraction could partially operate, as shown by a lower 1/n value for

376

the same components. The difference may be attributed to more operation of site-limiting

377

mechanism (i.e., electrostatic attraction) at pH 4.0. The different adsorption behaviors

378

between C1 and C2 were in a good agreement with a structural trend with the sizes of the

379

ultrafiltered fractions revealed by our 13C NMR results (Supplementary Information, Table

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14

ACCEPTED MANUSCRIPT S4), in which the larger sized fractions retain relatively high aromaticity and more abundant

381

carboxylic functional groups (i.e., more negatively charged). Comparison of the SEC

382

chromatograms before and after adsorption also supported the more site-limitation for

383

adsorption of the larger sized HA molecules as demonstrated by more adsorption of smaller

384

molecular sizes with a higher initial HA concentration (i.e., more competition)

385

(Supplementary Information, Fig S12).

386

388

3.7. Changes in C1/C2 ratios with adsorbed HS amount

Changes in the HA molecular sizes upon adsorption were tracked by the C1/C2 ratios

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387

SC

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380

against the amounts of adsorbed HA (Fig. 6c). Higher C1/C2 ratios of adsorbed HA were

390

consistently observed at pH 4.0 versus pH 6.0 for a range of the adsorption amounts,

391

indicating that preferential adsorption of C1 over C2 was more evident at pH 4.0. In detail,

392

the C1/C2 ratios were higher than the original value (1.01) at relatively low adsorbed HA

393

amounts (up to ~20 mgC/g), and they became similar to or lower than the original value as

394

the adsorbed HA amount increased. These results suggest that although preferential

395

adsorption of relatively large HS aromatic molecules occurred on the GO surface at the pH,

396

the degree became diminished as the available surface sites were occupied. At pH 6.0, the

397

C1/C2 ratios were mostly lower than the original value, implying that relatively smaller sized

398

aromatic molecules were more attractive to the GO surface. One exception was the lowest

399

adsorbed HA amount, in which the ratio was higher than the original value. Similarly to pH

400

4.0, the C1/C2 ratios showed a decreasing trend with increased adsorbed HA amount up to

401

~20 mgC/g, and they remained within a limited range above that range. Our results are in line

402

with a prior study of Yang and Xing (2009), who reported using a rough estimate of

403

molecular size based on an absorption ratio (i.e., UV250/UV365) that preferential adsorption of

404

larger molecular sized HS onto CNTs was more evident at a lower pH.

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15

ACCEPTED MANUSCRIPT 405

Taken together, our study demonstrated that the degree and the trend of HA size fractionation upon the adsorption onto GO surface can be highly dependent on the solution

407

pH and the available GO surface sites. Further investigation could provide more concrete

408

evidence for our explained mechanisms associated with the adsorptive fractionation.

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406

409 410

4. Conclusions

Adsorptive fractionation of HA on GO surface was confirmed by tracking the optical

412

properties of HA upon the adsorption. UV-absorbing HA molecules were preferentially

413

adsorbed onto GO at the two pH conditions, and they showed a faster adsorption rate

414

compared to the bulk HA. The aromatic HA moieties exhibited different adsorption behaviors

415

from the bulk HA, showing more linear isotherms and a higher Qmax and a lower kL values at

416

pH 4.0 than at pH 6.0. A positive relationship was established between the C1/C2 ratios and

417

MWw values of HA ultrafiltered size fractions, suggesting that EEM-PARAFAC could be

418

used for tracking the changes in the molecular sizes of HA. The two individual adsorption

419

isotherms of C1 and C2 revealed that the larger sized humic-like component (C1) had a

420

greater adsorption affinity but more limited adsorption sites on the GO surface. The observed

421

adsorption behaviors including the size fractionation were possibly explained by the relative

422

contributions of different mechanisms, the amount of adsorbed HA (i.e., available surface

423

sites), and a structural trend of HA with its fraction’s size.

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411

425

Acknowledgments

426

This work was supported by a National Research Foundation of Korea (NRF) grant funded

427

by the Korea government (MSIP) (No. 2014R1A2A2A09049496).

428 429

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Banaitis, M.R., Waldrip-Dail, H., Diehl, M.S., Holmes, B.C., Hunt, J.F., Lynch, R.P. and Ohno, T. (2006) Investigating sorption-driven dissolved organic matter fractionation by multidimensional fluorescence spectroscopy and PARAFAC. Journal of Colloid and Interface Science 304(1), 271-276.

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Cuss, C.W. and Guéguen, C. (2012) Determination of relative molecular weights of fluorescent components in dissolved organic matter using asymmetrical flow field-flow fractionation and parallel factor analysis. Analytica Chimica Acta 733, 98-102. Dainard P.G., Guéguen, C. (2013) Distribution of PARAFAC modeled CDOM components in the North Pacific Ocean, Bering, Chnkchi and Beaufort Seas. Marine Chemistry 157, 216223

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Tables Table 1. Isotherm model parameters of ESHA adsorption. Langmuir pH Qmax kL R2

UV

kF

1/nd

R2

4

47.9±4.1a

0.080±0.019b

0.91

8.43±1.77c

0.402±0.064

0.86

6

69.0±7.0a

0.019±0.003b

0.99

2.41±0.26c

0.680±0.031

0.99

4

710±290e

0.122±0.063f

0.96

77.56±4.09g

0.832±0.067

0.97

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DOC

Freundlich

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6 417±42e 0.167±0.023f 0.99 60.30±1.55g 0.771±0.029 0.99 a the maximum adsorption capacity estimated based on DOC measurement (mg C/g) b the adsorption affinity estimated based on DOC measurement (L/mg C) c the Freundlich model capacity estimated based on DOC measurement ((mg C/g)(L/mg)1/n) d the Freundlich intensity factor, an indicator of isotherm nonlinearity (dimensionless) e the maximum adsorption capacity estimated based on UV absorption measurement (1/cm·g) f the adsorption affinity estimated based on UV absorption measurement (cm) g the Freundlich model capacity estimated based on UV absorption measurement ((1/cm·g)(cm)1/n) h Not measured

DOC

a

AC C

UV

pH

Qe

kt

R2

4.0

16.67±0.27a

8.77±1.00b

0.96

6.0

7.73±0.26a

5.54±0.97b

0.87

4.0

0.821±0.016c

9.69±1.46b

1.00

6.0

c

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Measurements

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Table 2. Parameters for the pseudo first-order model.

0.618±0.007

22.03±9.73

b

Adsorbed amount in DOC concentrations at equilibrium condition (mg C/g) Pseudo first model constant (1/h) c Adsorbed amount in UV absorbance (at 254 nm) at equilibrium condition (1/cm·g) b

1.00

ACCEPTED MANUSCRIPT Table 3. Isotherm model parameters for each PARAFAC component.

4.0

6.0

Langmuir

comp-

Freundlich kF

1/ng

R2

0.97

7.34±0.52c

0.57±0.02

0.99

0.025±0.005b

0.98

5.22±0.52c

0.70±0.03

0.99

135±23a

0.017±0.004b

0.98

3.57±0.48c

0.74±0.04

0.98

a

b

0.99

c

0.81±0.04

0.99

onents

Qmax

kL

R

C1

87±8a

0.046±0.008b

C2

128±18a

C1 C2

187±29

0.013±0.003

a

2

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pH

3.36±0.40

the maximum adsorption capacity of PARAFAC components (QSE/g) the adsorption affinity of PARAFAC components (L/QSE) c the Freundlich constant of PARAFAC components ((QSE/g)(L/mg)1/n)

AC C

EP

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b

1

ACCEPTED MANUSCRIPT

45

(a)

ESHA pH 4.0

40

ESHA pH 6.0 Langmuir

35

Freundlich

25

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Q e (mg C/g)

30

20 15

5 0 10

20

30

40

M AN U

0

SC

10

50

Ce (mg C/L)

250 ESHA pH 4.0 ESHA pH 6.0 Langmuir Freundlich

TE D

150

100

AC C

50

EP

Qe (1/cm g)

200

(b)

0

0.0

0.5

1.0

1.5

2.0

2.5

3.0

3.5

Ce (1/cm)

Fig. 1. Adsorption isotherms of ESHA on GO at 0.1 M NaCl based on (a) DOC measurements and (b) UV absorption measurements (UV254).

1

ACCEPTED MANUSCRIPT

25 ESHA pH 4.0

(a)

ESHA pH 6.0

20

15

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Qt (mg C/g)

Pseudo first order

10

0 1

2

3

4

5

M AN U

0

SC

5

6

Adsorption time (hr)

1.0

TE D

0.6

0.4

ESHA pH 4.0

EP

Q t (1/cm g)

0.8

0.2

AC C

(b)

ESHA pH 6.0 Pseudo first order

0.0

0

1

2

3

4

5

6

Adsorption time (hr)

Fig. 2. Adsorption kinetics of ESHA on GO at 0.01 M NaCl based on (a) DOC measurements and (b) UV absorption measurements. Error bars represent triplicate samples. The composite samples were used for the absorption and the fluorescence measurements.

1

20

(a)

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18 16 14 12 10

SC

8 6

ESHA pH 4.0

4

ESHA pH 6.0

2

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SUVA values of adsorbed ESHA (L/mg C·m)

ACCEPTED MANUSCRIPT

ESHA

0 0

10

20

30

40

13

(b)

ESHA pH 4.0

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12 11

ESHA pH 6.0 ESHA

EP

10 9 8

AC C

SUVA values of adsorbed ESHA (L/mg C·m)

Adsorbed amount of ESHA (mg C/g)

7 6

0

1

2

3

4

5

6

Adsorption time (hr)

Fig. 3. Changes in the SUVA values of adsorbed ESHA with (a) adsorption amount at equilibrium condition and (b) adsorption times (adsorption kinetics).

1

ACCEPTED MANUSCRIPT 500

500

(a)

(b)

(C)

350

0 2e-2 3e-2 4e-2 5e-2 6e-2 7e-2

300

400

350 0 2e-2 3e-2 4e-2 5e-2 6e-2 7e-2

300

250 350

400

450

500

550

Emission (nm)

350

300

250 300

400

250 300

350

400

450

Emission (nm)

500

550

0 4.0e-2 6.0e-2 8.0e-2 1.0e-1 1.2e-1

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400

450

Excitation (nm)

450

Excitation (nm)

450

300

350

400

SC M AN U TE D EP 1

450

Emission (nm)

Fig. 4. PARAFAC components (a) C1, (b) C2, and (c) C3.

AC C

Excitation (nm)

500

500

550

ACCEPTED MANUSCRIPT

3.0 2.5

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C1/C2 ratios

2.0 1.5

SC

1.0

0.0 0

2000

M AN U

0.5

4000 MWW (Da)

6000

8000

Fig. 5. A relationship between the ratios of the two PARAFAC components (C1/C2) and

AC C

EP

TE D

weight-averaged molecular weights for five ultrafiltered size fractions of ESHA.

1

ACCEPTED MANUSCRIPT

70

(a) 60

40

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Qe (QSE/g)

50

30

C1

20

C2

SC

Langmuir

10

Freundlich

0 10

20

30

40

M AN U

0

Ce (QSE)

70

(b) 60

TE D

40 30

C1

EP

Qe (QSE/g)

50

20

C2 Langmuir

AC C

10

Freundlich

0

0

10

20 Ce (QSE)

1

30

40

ACCEPTED MANUSCRIPT

(c) 1.1

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1.0 0.9 0.8

ESHA pH 4.0

0.7

ESHA pH 6.0

0.6

SC

C1/C2 ratios of adsorbed ESHA

1.2

ESHA

10

20

30

M AN U

0

40

Adsorbed amount of ESHA (mg C/g)

Fig. 6. Adsorption isotherms of C1 and C2 at (a) pH 4.0 and (b) pH 6.0, and (c) changes of

AC C

EP

TE D

C1/C2 ratios of adsorbed ESHA with the adsorption amounts on GO.

2

ACCEPTED MANUSCRIPT

Highlights

► EEM-PARAFAC was successfully applied to examine HS adsorptive behavior on

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graphene oxide (GO).

SC

► Aromatic molecules within HS were preferentially adsorbed onto GO surface.

higher isotherm nonlinearity.

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► Larger sized fluorescent component exhibited a greater adsorption affinity and a

AC C

EP

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► Adsorptive fractionation depends on solution pH and available sites on GO.

ACCEPTED MANUSCRIPT

Supplementary Information Water Research

1 2 3 4 5

Investigation of adsorptive fractionation of humic acid on graphene oxide

7

using fluorescence EEM-PARAFAC

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6

8

b

Department of Environment and Energy, Sejong University, Seoul, 143-747, South Korea Department of Nano Materials Engineering, Sejong University, Seoul, 143-747, South Korea

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a

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Bo-Mi Leea, Young-Soo Seob, and Jin Hura,*

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* Corresponding author: Tel. +82-2-3408-3826. E-mail: [email protected]

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Fax +82-2-3408-4320.

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S1. Characterization of GO To confirm the synthesis of GO, the structural features of graphite and the synthesized GO were compared each other by employing a variety of the characterizing tools including

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scanning electron microscopy (SEM), atomic force microscopy (AFM), X-ray diffraction

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(XRD), Raman spectroscopy, and Fourier transform infrared spectroscopy (FTIR). It was

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clearly seen that the graphite retained stacked graphene layers, while the exfoliated GO was

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wrinkled in its thin layer (Fig. S1a). From the AFM scanning (Fig. S2), it was confirmed that

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our synthesized GO consists of the single layers with its thichness of approximately 1 nm.

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Similar GO structure with thin layers was also reported in other previous studies (Cote et al.,

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2009; Sun et al., 2012). The XRD spectrum of GO showed a prominant peak at lower degree

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at 10.82°. In contrast, there were two sharp peaks at 26.34° and 54.52° for graphite (Fig. S3).

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The peak at the lower degree is associated with longer distances between the atoms within the

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structures, suggesting that the the adjacent layers of the GO are placed in longer distances

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between one another than those of the graphite. For example, the degree of the GO peak

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corresponds to 0.822 nm while those of the graphite reflect 0.340 nm and 0.169 nm,

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respectively. Moon et al. also reported the similar results of 0.330 nm and 0.860 nm for

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graphite and GO, respectively (Moon et al., 2010).

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In the Raman spectra (Fig. S4), graphene peak (G peak at 1580 cm-1) and two-dimension

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peak (2D peak at 2700 cm-1) were observed for graphite, while the GO showed a defected

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peak (D peak at 1336 cm-1), the G peak, and an decresed 2D peak. The formation of D peak

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indicates that the sp2 structure may be partially defected by strong oxidation (Moon et al.,

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2010). However, the defection does not appear to be unsual because our defected rate (0.86)

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base on the relative intensities of the D peak to the G peak (ID/IG) fell within the range

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previously reported (Moon et al., 2010; Wang et al., 2014). According to Acik et al. (2010), 2

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the FT-IR peaks of GO are typically shown at the wavenumber ranges associated with the

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vibration of epoxide (C-O-C) (1230-1320 cm-1), sp2-hydridized C=C (1500-1600 cm-1),

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carboxyl (COOH) (1650-1750 cm-1), ketonic species (C=O) (1600-1650 cm-1, 1750-1850 cm-

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1

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similar peaks at 1134 cm-1, 1261 cm-1, 1408 cm-1, 1640 cm-1, 1731 cm-1, 3218 cm-1, and 3401

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cm-1 for the GO , indicating that the GO can be characterized by sp2 structure and the

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functional groups of epoxy, carboxy, and hydroxyl. The point of zero charge of the GO in this

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study was estimated to be 4.65 based on an acid-base titration (Fig. S6) (Zhao et al., 2012).

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), and hydroxyl (C-OH) (3050-3800 cm-1 and 1070 cm-1). Our FT-IR result showed the

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Fig. S1. Images of scanning electron microscopy (SEM) for (a) graphite and (b) GO.

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Fig. S2. AFM image of GO. 3

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10.82˚

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Arb. intensity

26.34˚

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GO

54.52˚

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30

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Graphite 60

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2 θ (°)

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Fig. S3. Comparison of the XRD images for graphite and GO in this study.

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2D-band

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Arb. intensity

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D-band G-band

500

1000

GO

Graphite 1500

2000

2500

3000

3500

Raman Shift (cm -1) 88 89

Fig. S4. Comparison of the Raman spectra for graphite and GO in this study. 4

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C-O-C

COOH

-OH

C=C

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Arb. intensity

C=O

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GO

Graphite

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Wavenumber (cm -1)

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Fig. S5. Comparison of the FT-IR spectra for graphite and GO in this study.

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Table S1. Calculated atomic distance of graphite and GO based on the XRD spectra. Graphite

95 96

54.52

10.82

0.34

0.17

0.82

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d (nm)

26.34

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2θ ( ˚ )

GO

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0.0015

0.0010

pHpzc=4.65

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0.0005

0.0000

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-0.0015 4

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pH

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Fig. S6. Acid-base titration curve for GO.

100 101

120 100.0

96.5

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Core consistency (%)

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60 40

17.7

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0.1 0 1 102 103

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3 Component No.

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Fig. S7. Result of core consistency test (n=46). 6

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Fig. S8. The split half test results as PARAFAC excitation and emission loadings of (a) C1, (b) C2 and (c) C3.

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Table S3. Adsorption model parameters for SRFA models

Isotherm

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Isotherm

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Freundlich

Kinetic 114 115 116 117 118 119 120 121 122

DOC measurements

UV254 measurements

Qmax

36.0±6.9a

-e

kL

0.010±0.002b

-e

R2

0.98

-e

kF

0.54±0.06c

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1/n

0.791±0.033d

-e

R2

0.99

-e

Qe

9.65±0.09f

0.383±0.011h

kt

5.77±0.36g

8.98±3.00g

Parameters

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Pseudo-first model

R2 0.97 0.99 a the maximum adsorption capacity estimated based on DOC measurement (mg C/g) b the adsorption affinity estimated based on DOC measurement (L/mg C) c the Freundlich model capacity estimated based on DOC measurement ((mg C/g)(L/mg)1/n) d the Freundlich intensity factor, an indicator of isotherm nonlinearity (dimensionless) e Not measured f Adsorbed amount in DOC concentrations at equilibrium condition (mg C/g) g Pseudo first model constant (1/h) h Adsorbed amount in UV absorbance (at 254 nm) at equilibrium condition (1/cm·g) 8

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S2. Ultrafiltration of ESHA and the characterization of the HS size fractions The chatacteristics of the five ultrafiltered size fractions of ESHA are presented in Table

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S2. The size fractions of > 30 kDa consititues nearly 88% of the total DOC pool of ESHA

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(Table S2). In general, the larger ultrafiltered fractions exhibited higher SUVA, higher

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aromaticity (aromatic carbon/aliphatic carbon), higher C1/C2 ratios, and more abaundance of

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carboxyl functional groups than smaller sized fractions (Table S2). A portion of the size

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exclusion (SEC) chromatograms of the different size fractions were overlapped with each

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other, but the size fractionation through the ultrafiltration processes could be confirmed by

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the shorter retention times of the highest peaks for the obtained size fractions in the order of

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under 1 kDa (10.27 min) > 1-10 kDa (9.73 min) > 10-30 kDa (9.33 min) > 30-100 kDa (8.92

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min) > over 100 kDa (6.03 min) (Fig. S7). In this study, the highest peak at humic-like

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fluroescence region of the excitation-emission spectra tends to be shifted toward longer

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wavelengths for larger ESHA sized fractions (Fig. S8). This osbservation agreed well with a

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previous report based on humic substances extracted from soils and sediments (Hur and Kim,

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2009). It was previously demonstrated that the red-shifting is typically associated with more

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condensed and polymerized structures of humic substances (Chen et al., 2003; Sierra et al.,

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2005).

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ACCEPTED MANUSCRIPT Table S4. Characteristics of different ultrafiltered size fractions of ESHA Distri-

SUVA

bution

(L/mg C-

(%)

m)

1>

2.93

3.69

1-10

1.29

10-30

Size

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MWw

C-NMR C1/C2

Carboxyl

Aliphatic C

Aromatic C

(%)

(%)

(%)

1105

9.4

40.2

47.3

1.18

0.23

7.00

1349

9.1

42.1

46.8

1.11

0.76

7.25

8.74

1883

11.4

33.8

51.7

1.53

1.56

30-100

30.5

9.51

3639

14.0

30.0

51.8

1.73

2.11

100 <

58.1

8.63

7165

13.2

30.4

52.5

1.73

2.46

(kDa)

(Da)

Aromaticity

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Note that the dissimilarity in the molecular weight values defined by the two fractionation methods (i.e., smaller MW for SEC vs. ultrafiltration) is attributed to the differences in the two systems including the molecular weight standard, separation principles, environmental conditions (Li et al., 2004).

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residual HS for adsorption kinetics.

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Table S4. Changes in the relative abundance of C1, C2, and C3 in the Fmax values (%) of

ESHA

4.0

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6.0

SRFA

4.0

%C1 48.0 43.9 42.9 42.6 42.9 42.3

Fmax constitution (%) %C2 47.5 44.7 46.8 46.9 46.9 47.8

%C3 5.0 13.9 11.7 11.5 11.3 10.8

0.0 0.2 0.5 1.0 2.0 5.0

48.0 33.4 34.8 34.4 33.9 34.1

47.5 59.0 59.7 57.6 58.3 58.3

5.0 6.7 4.8 7.2 7.0 6.7

0.0

6.6

68.8

24.6

0.3 0.6

5.9 5.2

67.6 73.4

26.5 21.4

1.1 2.1 5.0

9.7 5.8 5.7

68.9 72.7 72.8

21.4 21.6 21.5

adsorption time (hr) 0.0 0.2 0.5 1.0 2.0 5.0

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pH

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Table S5. Changes in the relative abundance of C1, C2, and C3 in the Fmax values (%) of

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residual ESHA for the adsorption isotherms.

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%C2 47.5 44.5 48.3 47.9 46.9 47.1 49.3 46.8 46.6 46.3 45.5 46.2 42.0 43.1 41.9 42.8 39.3 38.5 42.9 43.1 43.3 38.5 43.7

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%C3 5.0 19.2 7.3 5.9 5.3 6.4 6.4 5.8 5.0 5.5 6.0 4.6 18.4 13.8 14.8 12.0 17.3 19.8 10.9 10.7 8.9 19.8 9.9

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%C1 48.0 36.3 44.5 46.2 47.8 46.5 44.2 47.5 48.4 48.2 48.5 49.1 39.6 43.2 43.4 45.2 43.4 41.8 46.2 46.2 47.9 41.7 46.4

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Fmax constitution (%)

Initial conc. (mg C/L)

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0.0008 0.0006

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DOC-normalized UV signal (at 254 nm)

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100000

Molecular Weight (Da)

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Fig. S9. SEC chromatograms of different ultrafiltered size fractions (UV-D at 254 nm)

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Fig. S10. Fluorescence excitation-emission matrices of different ultrafiltered size fractions of

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(a) <1 kDa, (b) 1-10 kDa, (c) 10-30 kDa, (d) 30-100 kDa, and (e) >100 kDa. 13

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(a)

DOC

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Langmuir Freundlich

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Q e (mg C/g)

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Ce (mg C/L)

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Qt (mg C/g)

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UV at 254 nm

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Pseudo first order

0

0

1

Qt (1/cm·g)

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0.000 2

3

4

5

6

Adsorption time (hr)

170 171

Fig. S11. (a) Adsorption isotherms of SRFA by DOC measurements and (b) adsorption

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kinetic of SRFA by DOC measurements and UV absorption measurements (UV254) at pH 4.0.

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(The amount of GO used is 500 mg/L).

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Fig S12. Molecular weight distributions of adsorbed ESHA in percentages. (a) pH 4.0, (b) pH

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6.0. The samples were obtained from adsorption isotherm experiments. The numbers in the

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parentheses indicate the percent removals in DOC by adsorption. Please note that site-limited

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adsorption (or competition) is more pronounced with a higher concentration of the initial HA

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(or at a lower removal percentage).

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References

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Acik, M., Lee, G., Mattevi, C., Chhowalla, M., Cho, K. and Chabal, Y.J. (2010) Unusual infrared-absorption mechanism in thermally reduced graphene oxide. Nature Materials 9(10), 840-845.

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Chen, J., LeBoeuf, E.J., Dai, S. and Gu, B. (2003) Fluorescence spectroscopic studies of natural organic matter fractions. Chemosphere 50(5), 639-647.

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Cote, L.J., Kim, F. and Huang, J.X. (2009) Langmuir-Blodgett Assembly of Graphite Oxide Single Layers. Journal of the American Chemical Society 131(3), 1043-1049.

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Hur, J. and Kim, G. (2009) Comparison of the heterogeneity within bulk sediment humic substances from a stream and reservoir via selected operational descriptors. Chemosphere 75(4), 483-490.

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Li, L., Zhao, Z., Huang, W., Peng, P., Sheng, G. and Fu, J. (2004) Characterization of humic acids fractionated by ultrafiltration. Organic Geochemistry 35, 1025-1037. Moon, I.K., Lee, J., Ruoff, R.S. and Lee, H. (2010) Reduced graphene oxide by chemical graphitization. Nature Communications 1(73).

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Sun, W.L., Xia, J., Li, S. and Sun, F. (2012) Effect of natural organic matter (NOM) on Cu(II) adsorption by multi-walled carbon nanotubes: Relationship with NOM properties. Chemical Engineering Journal 200–202, 627-636.

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Sierra, M.M.D., Giovanela, M., Parlanti, E. and Soriano-Sierra, E.J. (2005) Fluorescence fingerprint of fulvic and humic acids from varied origins as viewed by single-scan and excitation/emission matrix techniques. Chemosphere 58(6), 715-733.

Wang, F., Haftka, J.J.H., Sinnige, T.L., Hermens, J.L.M. and Chen, W. (2014) Adsorption of polar, nonpolar, and substituted aromatics to colloidal graphene oxide nanoparticles. Environmental Pollution 186(0), 226-233.

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Zhao, G.X., Wen, T., Yang, X., Yang, S.B., Liao, J.L., Hu, J., Shao, D.D. and Wang, X.K. (2012) Preconcentration of U(VI) ions on few-layered graphene oxide nanosheets from aqueous solutions. Dalton Transactions 41(20), 6182-6188.

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